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Euclid Q1 catalogue covers 378,000 galaxies

Astronomy research
NASA, ESA, and The Hubble Heritage Team STScI/AURA), Wikimedia Commons, Public domain · Public domain

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What the study found

The study reports a detailed visual morphology catalogue for Euclid Quick Release 1, covering 378,000 bright or extended galaxies. The catalogue includes features such as bars, spiral arms, and ongoing mergers.

Why the authors say this matters

The authors say the measurements are fully automated and therefore fully scalable. They also note that this catalogue is the first 0.4% of the roughly 100 million galaxies in which Euclid will ultimately resolve detailed morphology.

What the researchers tested

The researchers created the catalogue by fine-tuning the Zoobot galaxy foundation models on annotations from a one-month campaign by Galaxy Zoo volunteers. They applied this approach to Euclid Quick Release 1 galaxy images.

What worked and what didn't

The abstract states that the catalogue was successfully produced and that the measurements are fully automated. It does not describe failures, comparisons, or performance limits.

What to keep in mind

The summary available here does not describe detailed validation, uncertainty, or limitations beyond the scope of the catalogue. It also covers only the Euclid Quick Release 1 sample described in the abstract.

Key points

  • A detailed visual morphology catalogue was produced for Euclid Quick Release 1.
  • The catalogue covers 378,000 bright or extended galaxies.
  • Galaxy features included bars, spiral arms, and ongoing mergers.
  • The catalogue was made by fine-tuning Zoobot models on Galaxy Zoo volunteer annotations.
  • The authors describe the measurements as fully automated and scalable.

Disclosure

Research title:
Euclid Q1 catalogue covers 378,000 galaxies
Authors:
Mike Walmsley, L. Quilley, Karen L. Masters, Sandor Kruk, K. A. Remmelgas, Jürgen Popp, E. Romelli, David O’Ryan, H. J. Dickinson, Chris Lintott, S. Serjeant, Rebecca Smethurst, Brooke Simmons, Jason Shingirai Makechemu, Izzy L. Garland, H. L. Roberts, Kameswara Bharadwaj Mantha, L. Fortson, Tobias Géron, William C. Keel, E. M. Baeten, C. Macmillan, Jo Bovy, Santiago Casas, C. De Leo, H. Domínguez Sánchez, J. Katona, J. H. Knapen, András Kovács, N. Aghanim, B. Altieri, A. Amara, S. Andreon, N. Auricchio, H. Aussel, C. Baccigalupi, Marco Baldi, A. Balestra, S. Bardelli, A. Basset, P Battaglia, R. Bender, A. Biviano, Andrea Bonchi, E. Branchini, M. Brescia, J. Brinchmann, S. Camera, G Cañas-Herrera, V. Capobianco, C. Carbone, J. Carretero, F. J. Castander, M. Castellano, G. Castignani, S. Cavuoti, K. C. Chambers, A Cimatti, C. Colodro-Conde, G. Congedo, Christopher J. Conselice, L. Conversi, Y. Copin, F. Courbin, H. M. Courtois, M. Cropper, A. Da Silva, H. Degaudenzi, G. De Lucia, A. M. Di Giorgio, C. Dolding, H. Dole, F. Dubath, C. A. J. Duncan, X. Dupac, S. Dusini, A. Ealet, S. Escoffier, Maximilian Fabricius, M. Farina, R. Farinelli, F Faustini, F. Finelli⋆, P. Fosalba, S. Fotopoulou, M. Frailis, E. Franceschi, S. Galeotta, Koshy George, B. Gillis, C. Giocoli, P. Gómez-Álvarez, J Gracia-Carpio, B. R. Granett, A. Grazian, F. Grupp, Stephen Gwyn, S. V. H. Haugan, Henk Hoekstra, W. Holmes, I. Hook, F. Hormuth, A. Hornstrup, P. Hudelot, K. Jahnkę, M. Jhabvala, Benjamin Joachimi, E. Keihänen, S. Kermiche, A. Kiessling, R. Kohley, B. Kubik, Konrad Kuijken, M Kümmel, M. Kunz, H. Kurki‐Suonio, O. Lahav, Q. Le Boulc’h, A.M.C Le Brun, D. Le Mignant, P. Liebing, S. Ligori, P. B. Lilje, V. Lindholm, I. Lloro, G Mainetti, D Maino, E. Maiorano, O. Mansutti, S. Marcin, O. Marggraf, M. Martinelli, N. Martinet, F. Marulli, R. Massey, S. Maurogordato, H. J. McCracken, E. Medinaceli, S. Mei, M. Melchior, Y Mellier, M. Meneghetti, E. Merlin, G. Meylan, A. Mora, M. Moresco, L. Moscardini, R. Nakajima, C. Neissner, R. C. Nichol, S.-M. Niemi, J.W Nightingale, C. Padilla Aranda, S. Paltani, F. Pasian, K. Pedersen, Will J. Percival, V. Pettorino, S. Pires, G. Polenta, M. Poncet, L. A. Popa, L. Pozzetti, F. Raison, R. Rébolo, A. Renzi, Jason Rhodes, G. Riccio, M. Roncarelli, B. Rusholme, R. P. Saglia, Z. Sakr, Ariel G. Sánchez, D. Sapone, B. Sartoris, J. A. Schewtschenko, Peter Schneider, T. Schrabback, M. Scodeggio, A. Secroun, G. Seidel, M. D. Seiffert, S. Serrano, P Simon, C. Sirignano, G. Sirri, L. Stančo, J. Steinwagner, P. Tallada-Crespí, D. Tavagnacco, A. J. Taylor, Harry I. Teplitz, I. Tereno, N Tessore, Sune Toft, R. Toledo-Moreo, F. Torradeflot, I. Tutusaus, E. A. Valentijn, L. Valenziano, J. Väliviita, T. Vassallo, G. Verdoes Kleijn, A. Veropalumbo, Yun Wang, J. Weller, A. Zacchei, G. Zamorani, F. M. Zerbi, I. A. Zinchenko, E. Zucca, V. Allevato, M. Ballardini, M. Bolzonella, E. Bozzo, C. Burigana, R. Cabanac, A. Cappi, D. Di Ferdinando, J. A. Escartin Vigo, L. Gabarra, J Martín-Fleitas, S Matthew, N. Mauri, R. B. Metcalf, A Pezzotta, M. Pöntinen, C. Porciani, I Risso, V. Scottez, M. Sereno, M. Tenti, Matteo Viel, M. Wiesmann, Y. Akrami, I.T Andika, S Anselmi, M. Archidiacono, F. Atrio‐Barandela, C. Benoist, K. Benson, Daniele Bertacca, M. Béthermin, G. Rodighiero, Alain Blanchard, L Blot, H. Böhringer, Michael D. Brown, S Bruton, F. Buitrago, Antonello Calabrò, B. Camacho Quevedo, F. Caro, C. S. Carvalho, T. Castro, F Cogato, Asantha Cooray, O. Cucciati, S. Davini, F. De Paolis, G. Desprez, A. Díaz‐Sánchez, J. J. Diaz, S. Di Domizio, J. M. Diego, Pierre–Alain Duc, A Enia, Y D Fang, A.G Ferrari, A. Finoguenov, A. Fontana, A Franco, K. Ganga, J. García-Bellido, T Gasparetto, V. Gautard, E. Gaztañaga, F. Giacomini, G. Gozaliasl, M Guidi, C. M. Gutiérrez, A Hall, W G Hartley, Shoubaneh Hemmati, C. Hernández–Monteagudo, H. Hildebrandt, J. Hjorth, J. J. E. Kajava, Y Kang, V. Kansal, D. Karagiannis, K Kiiveri, C. C. Kirkpatrick, J Le Graet, L. Legrand, Maria Lembo, Francesca Lepori, Gavin Leroy, G. F. Lesci, Julien Lesgourgues, L. Leuzzi, T.I Liaudat, A. Loureiro, J. F. Macías–Pérez, G. Maggio, M. Magliocchetti, F. Mannucci, R. Maoli, C. J. A. P. Martins, L. Maurin, M. Miluzio, Pierluigi Monaco, Claudio Moretti, G. Morgante, C Murray, S. Nadathur, Krishna Naidoo, A Navarro-Alsina, Savvas Nesseris, F. Passalacqua, K. Paterson, L. Patrizii, Alice Pisani, D. Potter, S Quai, M. Radovich, P.-F. Rocci, G. Rodighiero, S Sacquegna, M Sahlén, D. B. Sanders, E Sarpa, Claudia Scarlata, Joop Schaye, Aurel Schneider, M. Schultheis, D Sciotti, E. Sellentin, Francesco Shankar, Leigh C. Smith, G. Testera, G. Testera, Romain Teyssier, S. Tosi, A. Troja, M. Tucci, C. Valieri, A. Venhola, D. Vergani, G Verza, P Vielzeuf, N. A. Walton, É. Soubrié, D. Scott
Institutions:
Aalto University, Aix-Marseille Université, Aix-Marseille Université, Aix-Marseille Université, Aix-Marseille Université, Aix-Marseille Université, Aix-Marseille Université, Aix-Marseille Université, Aix-Marseille Université, ARC Centre of Excellence for Dark Matter Particle Physics, Arcetri Astrophysical Observatory, Astronomical Institute of the Slovak Academy of Sciences, Astronomical Institute of the Slovak Academy of Sciences, Astronomical Institute of the Slovak Academy of Sciences, Astronomical Institute of the Slovak Academy of Sciences, Astronomical Observatory of Capodimonte, Astronomical Observatory of Capodimonte, Astronomical Observatory of Capodimonte, Astronomical Observatory of Capodimonte, Astronomical Observatory of Rome, Astronomical Observatory of Rome, Astronomical Observatory of Rome, Astronomical Observatory of Rome, Astronomical Observatory of Rome, Astronomical Observatory of Rome, Astronomical Observatory of Rome, Astronomical Observatory of Rome, Astronomical 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Centre de physique des particules de Marseille, Centre de physique des particules de Marseille, Centre de Recherche Astrophysique de Lyon, Centre for Theoretical Physics and Astrophysics, Centre National d'Études Spatiales, Centre National d'Études Spatiales, Centre National de la Recherche Scientifique, Centre National de la Recherche Scientifique, Centre National de la Recherche Scientifique, Centre National de la Recherche Scientifique, Centre National de la Recherche Scientifique, Centre National de la Recherche Scientifique, Centre National de la Recherche Scientifique, Centre National de la Recherche Scientifique, Centre National de la Recherche Scientifique, Centre National de la Recherche Scientifique, Centre National de la Recherche Scientifique, Centre National de la Recherche Scientifique, Centre National de la Recherche Scientifique, Centre National de la Recherche Scientifique, Centre National de la Recherche Scientifique, Centre National de la Recherche Scientifique, 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Computing Center, Consejo Superior de Investigaciones Científicas, DAWN Center for Independent Living, DAWN Center for Independent Living, Durham University, École Normale Supérieure de Lyon, École Polytechnique Fédérale de Lausanne, Engineering Science Analysis (United States), Engineering Science Analysis (United States), Engineering Science Analysis (United States), Engineering Science Analysis (United States), Engineering Science Analysis (United States), Engineering Science Analysis (United States), Engineering Science Analysis (United States), Engineering Science Analysis (United States), Eötvös Loránd University, European Space Agency, European Space Agency, European Space Agency, European Space Agency, European Space Agency, European Space Agency, European Space Agency, European Space Agency, European Space Agency, European Space Agency, European Space Agency, European Space Research and Technology Centre, European Space Research and Technology Centre, European Space Research 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Publication date:
2026-06-30
DOI:
10.1051/0004-6361/202555140
OpenAlex record:
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Image credit:
NASA, ESA, and The Hubble Heritage Team STScI/AURA), Wikimedia Commons, Public domain
AI provenance: This post was generated by gpt-5.4-mini (OpenAI). The original authors did not write or review this post.

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